Zobrazeno 1 - 10
of 261
pro vyhledávání: '"Neta A Bahcall"'
Autor:
C. Sifon, Neta A. Bahcall, Jenny E. Greene, Ananth Tenneti, Andrew Hearin, Peter Behroozi, Felipe Ardila, Song Huang, Christopher Bradshaw, Kevin Bundy, Joshua S. Speagle, Alexie Leauthaud
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 492:3685-3707
Using deep images from the Hyper Suprime-Cam (HSC) survey and taking advantage of its unprecedented weak lensing capabilities, we reveal a remarkably tight connection between the stellar mass distribution of massive central galaxies and their host da
Autor:
Adam Burrows, Neta A. Bahcall
Publikováno v:
Proc Natl Acad Sci U S A
The 2019 Nobel Prize in Physics honors three pioneering scientists for their fundamental contributions to basic cosmic questions - Professor James Peebles (Princeton University), Michel Mayor (University of Geneva), and Didier Queloz (University of G
Autor:
Neta A. Bahcall
Publikováno v:
Nature Astronomy. 5:428-429
Autor:
Neta A. Bahcall, Yen-Chi Chen, Rachel Mandelbaum, Christopher R. Genovese, Donald P. Schneider, Peter E. Freeman, Larry Wasserman, Shirley Ho, Joel R. Brownstein
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 466:1880-1893
We study the effects of filaments on galaxy properties in the Sloan Digital Sky Survey (SDSS) Data Release 12 using filaments from the `Cosmic Web Reconstruction' catalogue (Chen et al. 2016), a publicly available filament catalogue for SDSS. Since f
Autor:
Robert H. Lupton, Yipeng Jing, Jiaxin Han, Paul A. Price, Alessandro Sonnenfeld, Eli S. Rykoff, Neta A. Bahcall, Masahiro Takada, Naoki Yasuda, Song Huang, Wentao Luo, Surhud More, Wenting Wang, Ting-Wen Lan, David V. Stark, Yutaka Komiyama, Xiangchong Li
Publikováno v:
Monthly Notices of the RAS (0035-8711), 487(2), 1580-1606
We study the faint stellar halo of isolated central galaxies, by stacking galaxy images in the HSC survey and accounting for the residual sky background sampled with random points. The surface brightness profiles in HSC $r$-band are measured for a wi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::da4ad56042bed0a338f12a6c6087d4d5
http://arxiv.org/abs/1811.04714
http://arxiv.org/abs/1811.04714
Publikováno v:
Solar Neutrinos ISBN: 9780429502811
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::11f6c4890425643357ebed5cc9ef5ddf
https://doi.org/10.1201/9780429502811-18
https://doi.org/10.1201/9780429502811-18
Autor:
Keiichi Umetsu, Atsushi J. Nishizawa, Elinor Medezinski, David N. Spergel, Masamune Oguri, Yen-Ting Lin, Nicholas Battaglia, Neta A. Bahcall, I. Non Chiu, Yutaka Komiyama, Cristóbal Sifón, Hironao Miyatake
Publikováno v:
Publications of the Astronomical Society of Japan. 70
Using $\sim$140 deg$^2$ Subaru Hyper Suprime-Cam (HSC) survey data, we stack the weak lensing (WL) signal around five Planck clusters found within the footprint. This yields a 15$\sigma$ detection of the mean Planck cluster mass density profile. The
Autor:
Takahiro Nishimichi, Atsushi J. Nishizawa, Masahiro Takada, Satoshi Miyazaki, Hung-Yu Jian, Yutaka Komiyama, Lihwai Lin, Rachel Mandelbaum, Neta A. Bahcall, Hironao Miyatake, Masamune Oguri, Yen-Ting Lin, Masayuki Tanaka, Song Huang, Taira Oogi, Jean Coupon, Masahiro Nagashima, Alexie Leauthaud, Surhud More
We present a statistical study of the redshift evolution of the cluster galaxy population over a wide redshift range from 0.1 to 1.1, using $\sim 1900$ optically-selected CAMIRA clusters from $\sim 232$~deg$^2$ of the Hyper Suprime-Cam (HSC) Wide S16
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3d551c7ee1871967f8a072fcabf29981
http://arxiv.org/abs/1709.01136
http://arxiv.org/abs/1709.01136
Autor:
Francisco-Shu Kitaura, Martin White, Rita Tojeiro, Chia-Hsun Chuang, Daniel Thomas, Shadab Alam, Jan Niklas Grieb, Florian Beutler, Hee-Jong Seo, Matthew D. Olmstead, Shirley Ho, Salvador Salazar-Albornoz, Ariel G. Sánchez, Joel R. Brownstein, Will J. Percival, Daniel J. Eisenstein, Siddharth Satpathy, Neta A. Bahcall, Jeremy L. Tinker
Publikováno v:
Satpathy, S, Alam, S, Ho, S, White, M, Bahcall, N A, Beutler, F, Brownstein, J R, Chuang, C-H, Eisenstein, D J, Grieb, J N, Kitaura, F, Olmstead, M D, Percival, W J, Salazar-Albornoz, S, Sánchez, A G, Seo, H-J, Thomas, D, Tinker, J L & Tojeiro, R 2017, ' The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey : On the measurement of growth rate using galaxy correlation functions ', Monthly Notices of the Royal Astronomical Society . https://doi.org/10.1093/mnras/stx883
Monthly Notices of the Royal Astronomical Society, vol 469, iss 2
Satpathy, S, Alam, S, Ho, S, White, M, Bahcall, N A, Beutler, F, Brownstein, J R, Chuang, C-H, Eisenstein, D J, Grieb, J N, Kitaura, F-S, Olmstead, M D, Percival, W J, Salazar-Albornoz, S, Sánchez, A G, Seo, H-J, Thomas, D, Tinker, J L & Tojeiro, R 2017, ' The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey : on the measurement of growth rate using galaxy correlation functions ', Monthly Notices of the Royal Astronomical Society, vol. 469, no. 2, pp. 1369-1382 . https://doi.org/10.1093/mnras/stx883
Satpathy, S; Alam, S; Ho, S; White, M; Bahcall, NA; Beutler, F; et al.(2017). The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: On the measurement of growth rate using galaxy correlation functions. Monthly Notices of the Royal Astronomical Society, 469(2), 1369-1382. doi: 10.1093/mnras/stx883. UC Berkeley: Retrieved from: http://www.escholarship.org/uc/item/1110v59w
Monthly Notices of the Royal Astronomical Society, vol 469, iss 2
Satpathy, S, Alam, S, Ho, S, White, M, Bahcall, N A, Beutler, F, Brownstein, J R, Chuang, C-H, Eisenstein, D J, Grieb, J N, Kitaura, F-S, Olmstead, M D, Percival, W J, Salazar-Albornoz, S, Sánchez, A G, Seo, H-J, Thomas, D, Tinker, J L & Tojeiro, R 2017, ' The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey : on the measurement of growth rate using galaxy correlation functions ', Monthly Notices of the Royal Astronomical Society, vol. 469, no. 2, pp. 1369-1382 . https://doi.org/10.1093/mnras/stx883
Satpathy, S; Alam, S; Ho, S; White, M; Bahcall, NA; Beutler, F; et al.(2017). The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: On the measurement of growth rate using galaxy correlation functions. Monthly Notices of the Royal Astronomical Society, 469(2), 1369-1382. doi: 10.1093/mnras/stx883. UC Berkeley: Retrieved from: http://www.escholarship.org/uc/item/1110v59w
We present a measurement of the linear growth rate of structure, \textit{f} from the Sloan Digital Sky Survey III (SDSS III) Baryon Oscillation Spectroscopic Survey (BOSS) Data Release 12 (DR12) using Convolution Lagrangian Perturbation Theory (CLPT)
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fbea81a142ad996d6c9e504a5d1fee19
https://www.pure.ed.ac.uk/ws/files/93485248/RSD_CLPT_DR12.pdf
https://www.pure.ed.ac.uk/ws/files/93485248/RSD_CLPT_DR12.pdf